Published September 1977
| Version v1
Journal article
Appearance of radiowave type 2 radiations in evolution of solar radio burst
Description
Studied is a relationship between the initial of radioemission generated by a coronal shock wave, and the time of a maximum intensity of the Hsub(α) line for flares giving rise to high-energy particles. Radioemission on the 2 type is shown to be mainly generated during the explosion phase of the flare of 00 maximum in the Hsub(α) line or in close vicinity theoreto
Additional details
Additional titles
- Original title (Russian)
- Появление радиоизлучения 2 типа в развитии солнечной радиовспышки
Publishing Information
- Journal Title
- Izv. Akad. Nauk SSSR, Ser. Fiz.
- Journal Volume
- 41
- Journal Issue
- 9
- Series
- Izv. Akad. Nauk SSSR, Ser. Fiz.
- Journal Page Range
- 1861-1863
- ISSN
- 0367-6765
Conference
- Title
- 8. International seminar on active processes on the Sun and solar neutrino problems.
- Dates
- 25 - 27 Sep 1976.
- Place
- Leningrad, USSR.
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 10453655
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BRIGHTNESS; RADIOWAVE RADIATION; SHOCK WAVES; SOLAR RADIO BURSTS; TIME DEPENDENCE
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SOLAR ACTIVITY
Optional Information
- Notes
- For English translation see the journal Bull. Acad. Sci. USSR, Phys. Sci.